Redshift Surveys and the Value of Omega

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dc.creatorFeldman, Hume A.
dc.creatorMelott, Adrian L.
dc.date1999-08-31
dc.date.accessioned2026-07-07T02:32:58Z
dc.date.available2026-07-07T02:32:58Z
dc.descriptionWe compare the statistical properties of structures normal and transverse to the line of sight which appear in observational data from redshift surveys. We present a statistic which can quantify this effect in a conceptually different way from standard analyses of distortions of the power-spectrum or correlation function. From tests with N-body experiments, we argue that this statistic represents a new, more direct and potentially powerful diagnostic of the cosmological density parameter Omega.
dc.description7 pages Latex, with 3 embedded figures. Uses paspconf.sty. To appear in the proceedings of the Cosmic Flows Workshop, Victoria, Canada, July 1999, ed. S. Courteau, M. Strauss & J. Willick, ASP series
dc.identifierhttps://arxiv.org/abs/astro-ph/9908352
dc.identifierhttp://arxiv.org/abs/astro-ph/9908352
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14662
dc.subjectAstrophysics
dc.titleRedshift Surveys and the Value of Omega
dc.typetext

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